The Northern Lights offer a bright spectacle during your late-night scrolling. Many planets, including Earth, have a magnetosphere—a vast magnetic shield created by the movement of the molten metal core extending into space.
Earth's magnetosphere protects us from harmful charged particles in space by absorbing their energy when they collide with it. When parts of this shield get overloaded with energy, a geomagnetic storm can develop, similar to how storm clouds gather before rain.
During these storms, stored energy flows along Earth's magnetic field lines and descends into the atmosphere like a heavy rain. This particle influx injects millions of amps into the atmosphere, producing brilliant auroral displays often visible far from the poles.
Occasionally, the Sun experiences magnetic storms that eject massive amounts of solar material into its atmosphere in explosive bursts. These large expulsions are known as coronal mass ejections (CMEs), appearing as enormous blobs moving through space.
The vibrant colors of auroras come from energetic particles striking gases in the upper atmosphere, with each gas producing unique colors at varied heights:
"The particle precipitation during geomagnetic storms injects millions of amps into the atmosphere, creating spectacular auroral displays far from the poles."
This fascinating dance of particles and atmospheric gases creates the captivating auroral shows that light up the night sky.
Author's summary: Earth's magnetic shield transforms solar energy into dazzling auroras, enchanting watchers with shifting colors from energetic particle collisions high in the atmosphere.